Bibcode
DOI
Pietarila, A.; Socas-Navarro, H.; Bogdan, T.; Carlsson, M.; Stein, R. F.
Referencia bibliográfica
The Astrophysical Journal, Volume 640, Issue 2, pp. 1142-1152.
Fecha de publicación:
4
2006
Revista
Número de citas
14
Número de citas referidas
10
Descripción
The Ca II infrared triplet lines around 8540 Å are good candidates
for observing chromospheric magnetism. Model spectra of these lines are
obtained by combining a radiation hydrodynamic simulation with a Stokes
synthesis code. The simulation shows interesting time-varying behavior
of the Stokes V profiles as waves propagate through the formation region
of the lines. Disappearing and reappearing lobes in the Stokes V
profiles as well as profile asymmetries are closely related to the
atmospheric velocity gradients.